中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Pulsar Pulse Nulling Fraction and Emission Height

文献类型:期刊论文

作者Yuen, Rai1,2,3,4,5
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2025-11-01
卷号25期号:11页码:115004
关键词stars: neutron (stars:) pulsars: general radiation mechanisms: non-thermal
ISSN号1674-4527
DOI10.1088/1674-4527/adfb4a
产权排序1
英文摘要We investigate the correlations between radio pulse nulling fraction (NF) and emission height based on simulation of 9000 nulling pulsar samples each with 1000 rotations. Each pulsar is randomly assigned an obliquity and a viewing angle. Visible emission is determined in a geometry, in which the emission is tangential to the local magnetic field lines and aligned with the line of sight. In an emission region with multiple emission segments, a detectable null occurs when a favorable condition is present to trigger switching in plasma density to zero in all the visible segments. The resulting NF distribution is consistent with the latest observations. We find that pulsars with low NFs and large obliquity angles tend to emit from higher heights, and vice versa. We demonstrate that variation in the NF is large among pulsars with low emission heights. However, the variation decreases and the NFs tend to be low for pulsars with emission at higher heights. We show that the NF exhibits varying correlation with the rotation period. Our results indicate that younger pulsars tend to null at higher emission heights than older pulsars. This suggests weakening of the radio emission mechanism with height as a pulsar ages.
WOS关键词RADIO-EMISSION ; DRIFTING SUBPULSES ; INTENSITY MEASUREMENTS ; PAIR PRODUCTION ; POLAR CAPS ; MODEL ; POLARIZATION ; PLASMA ; MAGNETOSPHERE ; ALTITUDE
资助项目National Natural Science Foundation of China (NSFC)[12288102] ; National Key Program for Science and Technology Research and Development[2022YFC2205201] ; National SKA Program of China[2020SKA0120200] ; National Natural Science Foundation of China (NSFC) project[12041303] ; National Natural Science Foundation of China (NSFC) project[12041304] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-2] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001574445500001
出版者IOP Publishing Ltd
资助机构National Natural Science Foundation of China (NSFC) ; National Key Program for Science and Technology Research and Development ; National SKA Program of China ; National Natural Science Foundation of China (NSFC) project ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China
源URL[http://ir.xao.ac.cn/handle/45760611-7/8154]  
专题脉冲星研究团组
通讯作者Yuen, Rai
作者单位1.State Key Lab Radio Astron & Technol, Beijing 100101, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Univ Sydney, Sch Phys, SIfA, Sydney, NSW 2006, Australia
4.Chinese Acad Sci, Key Lab Radio Astron & Technol, Beijing 100101, Peoples R China
5.Chinese Acad Sci, Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China
推荐引用方式
GB/T 7714
Yuen, Rai. Pulsar Pulse Nulling Fraction and Emission Height[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2025,25(11):115004.
APA Yuen, Rai.(2025).Pulsar Pulse Nulling Fraction and Emission Height.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,25(11),115004.
MLA Yuen, Rai."Pulsar Pulse Nulling Fraction and Emission Height".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 25.11(2025):115004.

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